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MCG-03-34-064

Observation

Spectrum ID105652557_sp1
Alt nameg1322245-164342
z0.0169
RA, Dec200.6019, -16.7285
MJD60352.75
SNR/Å B/R4.9/7.7
Obs Airmass1.03
SMSS ID105652557
Closest SMSS7.51'', 2172048483
SMSS Mean r6"ap13.9 ± 0.0
2MASS Kext9.7 ± 0.0

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.067
Power law αν-1.38 ± 0.50
log L5100,AGN42.60 ± 0.20
log HβBr/[O III]-1.32 ± 0.16
log ML5100/M6.61 ± 0.15
log M/M7.16 ± 0.04
log M/M6.61 ± 0.15
log M[O III]/M7.38 ± 0.12

Spatial extraction & sky subtraction region

Spatial plot

Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)

Spectrum decomposition

Emission line measurements

Linelog L (erg s⁻¹)FWHM (km s⁻¹)σ (km s⁻¹)EW (Å)
Hγ Narrow40.21 ± 0.33856 ± 97417 ± 4819.17 ± 5.49
Hγ Broad40.59 ± 0.171190 ± 65427 ± 2537.84 ± 5.97
[O III] 436440.12 ± 0.21486 ± 68205 ± 2815.53 ± 3.71
He II Narrow40.11 ± 0.25486 ± 68205 ± 2815.86 ± 3.46
He II Broad40.49 ± 0.181597 ± 128678 ± 5438.86 ± 5.98
Hβ Narrow40.81 ± 0.14856 ± 97417 ± 4881.73 ± 5.22
Hβ Broad40.83 ± 0.161419 ± 186564 ± 9977.09 ± 6.87
[O III] 500742.15 ± 0.02856 ± 97417 ± 481826.38 ± 9.67
He I Narrow39.93 ± 0.28486 ± 68205 ± 2811.93 ± 2.91
He I Broad40.13 ± 0.361694 ± 74719 ± 3018.82 ± 5.40
[O I] 630040.66 ± 0.06486 ± 68205 ± 2868.40 ± 3.60
Hα Narrow41.15 ± 0.05486 ± 68205 ± 28218.82 ± 6.51
Hα Broad41.99 ± 0.022136 ± 85779 ± 301437.71 ± 9.75
[N II] 658541.46 ± 0.03486 ± 68205 ± 28445.07 ± 6.30
[S II] 671840.89 ± 0.03486 ± 68205 ± 28121.06 ± 4.16
[S II] 673240.95 ± 0.03486 ± 68205 ± 28138.53 ± 4.23

All narrow line widths are tied to narrow [O III] 5007Å. [O III] 5007Å and narrow Hβ include a second narrow component not tied to other narrow lines.

Emission summary

Hα Broad SNR18.26
Hβ Broad SNR2.36
Hγ Broad SNR1.93
AGN frac0.17
Host frac0.83
log L5100,Host43.30
Fe II/Hβ1.12
Fe II/[O III]0.05

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer1
balmer_snr1
hb_width0
balmer_width2

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.